Journal
PHYSICS OF FLUIDS
Volume 15, Issue 2, Pages 315-329Publisher
AMER INST PHYSICS
DOI: 10.1063/1.1532731
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The objective of the present study is to analyze our recent direct numerical simulation (DNS) results to explain in some detail the main physical mechanisms responsible for the modification of isotropic turbulence by dispersed solid particles. The details of these two-way coupling mechanisms have not been explained in earlier publications. The present study, in comparison to the previous DNS studies, has been performed with higher resolution (Re-lambda=75) and considerably larger number (80 million) of particles, in addition to accounting for the effects of gravity. We study the modulation of turbulence by the dispersed particles while fixing both their volume fraction, phi(v)=10(-3), and mass fraction, phi(m)=1, for three different particles classified by the ratio of their response time to the Kolmogorov time scale: microparticles, tau(p)/tau(k)<1, critical particles, τ(p)/τ(k)≈1, large particles, τ(p)/τ(k)>1. Furthermore, we show that in zero gravity, dispersed particles with τ(p)/τ(k)=0.25 (denoted here as ghost particles) modify the spectra of the turbulence kinetic energy and its dissipation rate in such a way that keeps the decay rate of the turbulence energy nearly identical to that of particle-free turbulence, and thus the two-way coupling effects of these ghost particles would not be detected by examining only the temporal behavior of the turbulence energy of the carrier flow either numerically or experimentally. In finite gravity, these ghost particles accumulate, via the mechanism of preferential sweeping resulting in the stretching of the vortical structures in the gravitational direction, and the creation of local gradients of the drag force which increase the magnitudes of the horizontal components of vorticity. Consequently, the turbulence becomes anisotropic with a reduced decay rate of turbulence kinetic energy as compared to the particle-free case. (C) 2003 American Institute of Physics.
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